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• W1963771752 abstract "One of the major criticisms of identifying the infrared emission bands with polycyclic aromatic hydrocarbon (PAH) molecules has been the lack of a match between laboratory spectra of individual PAHs and the emission features. Part of the difficulty arises from the complexity of modeling the emission mechanism with an a priori unknown mixture of ionized and neutral PAHs. A direct comparison between laboratory spectra of PAHs and astronomical sources is possible for absorption spectra. However, because of poor atmospheric transmission, ground-based spectra of the PAH absorption band in the C-H stretch region are too noisy to make a detailed comparison with laboratory spectra. In this paper we show that ISO Short Wavelength Spectrometer spectra of a few protostars that show a 3.25 μm absorption band can be well matched by laboratory absorption spectra of a mixture of isolated PAHs." @default.
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• W1963771752 date "2001-06-10" @default.
• W1963771752 modified "2023-09-24" @default.
• W1963771752 title "Gas‐Phase Polycyclic Aromatic Hydrocarbons in Absorption toward Protostellar Sources?" @default.
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• W1963771752 doi "https://doi.org/10.1086/321347" @default.
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